The energy balance equation for a general solar atmosphere without assuming the planeparallel approximation is solved analytically. This leads to models for both the transition region and inner corona as well as for the outer corona. The form of the latter is very similar to that of the hydrostatic
โฆ LIBER โฆ
Temperature in transition region and inner corona
โ Scribed by Suresh Chandra
- Publisher
- Springer Netherlands
- Year
- 1983
- Tongue
- English
- Weight
- 71 KB
- Volume
- 96
- Category
- Article
- ISSN
- 0004-640X
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